We have collected several samples of disk galaxies, in order to study, in each of them, the relation between the blue total corrected absolute magnitude and the absolute corrected isophotal diameter. These Luminosity-Diameter relations have been compared, in order to detec a possible dependence on the density of the galaxy envionment. No significant differences have been found among the several relations, especially if selection criteria relative to the various samples are taken into account. The result is in disagreement with several previous claims.

Environment and the luminosity -diameter relation for disk galaxies

GIRARDI, MARISA;GIURICIN, GIULIANO;MARDIROSSIAN, FABIO;MEZZETTI, MARINO
1991

Abstract

We have collected several samples of disk galaxies, in order to study, in each of them, the relation between the blue total corrected absolute magnitude and the absolute corrected isophotal diameter. These Luminosity-Diameter relations have been compared, in order to detec a possible dependence on the density of the galaxy envionment. No significant differences have been found among the several relations, especially if selection criteria relative to the various samples are taken into account. The result is in disagreement with several previous claims.
2863320947
http://adsabs.harvard.edu/abs/1991phco.conf..452G
http://books.google.it/books?id=eT8VJXYQtnkC&printsec=frontcover&hl=it#v=onepage&q&f=false
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Utilizza questo identificativo per citare o creare un link a questo documento: http://hdl.handle.net/11368/2634677
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